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Line Formation in Moving Atmospheres
Published online by Cambridge University Press: 08 February 2017
Abstract
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We discuss an integral equation method that permits the calculation of the line source functions and of the emergent profiles in finite and semiinfinite atmospheres with macroscopic motion normal to the surface. Solutions are presented for a semiinfinite atmosphere with a temperature rise in the outward direction and with a flow that decays with increasing depth. The computed profiles have the form of P Cygni lines.
- Type
- Part B. Theoretical Methods for Handling Non-LTE Problems
- Information
- International Astronomical Union Colloquium , Volume 2: Spectrum Formation in Stars With Steady-State Extended Atmospheres , August 1970 , pp. 120 - 133
- Copyright
- Copyright © 1970
References
Hummer, D. G., and Rybicki, G. B.
1968, Proc. Conf. on Resonance. Lines in Astrophys., National Center for Atmospheric Research.Google Scholar
Jones, H. P., and Skumanich, A.
1968, Proc. Conf. on Resonance. Lines in Astrophys., National Center for Atmospheric Research.Google Scholar
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